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Habitability
11/ 100
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orbitar
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is a gas giant based of iau name (42 draconis b) and also is a 0.94 jupiter mass gas planet almost like jupiter but tilted due to a major collision in the past and also it had 6 moons one of them had life on the surface and also is a base for of my habitable worlds of this planet
Gas Giant
✦ cafarnaMagnetic FieldExtreme Activity
Why is this a Gas Giant?
Your planet has 69.1% hydrogen and helium, combined with a mass of 300.0x Earth, which exceeds the gas giant threshold.Gas giants form when massive cores capture enormous atmospheres of light gases. They typically form beyond the 'frost line' where volatiles can condense.
Classification Criteria:
✓ Hydrogen + Helium: 69.1% (>60% required)✓ Mass: 300.0x Earth (>10x required)
Habitability ScoreUninhabitable
Contributing Factors
water15
No solid surface — any water is locked in a supercritical mantle and hot ice, not oceans
geology40
Extreme volcanic activity may be hazardous
rotation10
Near tidally locked - one hemisphere perpetually scorched, other frozen, narrow habitable twilight zone only
Organic Chemistry84
Core organic elements (CHNO) present (tidal pools cycle wet and dry - a boost for prebiotic chemistry)
atmosphere12
Hydrogen-rich atmosphere typical of gas giants (partially stripped by slow rotation)
temperature20
Very cold - water frozen, challenging for life (extreme seasons: at 75° the poles swing between months-long day and night: −16% habitability)
magnetic Field100
Magnetic field provides radiation protection
Physical Properties
Mass
300.00x Earth (1.79e+27 kg)Radius
6.69x Earth (42,650 km)Surface Gravity
6.69x Earth (65.7 m/s²)Surface Temperature
145 K (-128 °C / -199 °F)Rotation Period
10.0 hours/day (faster than Earth)Orbital Environment
Star Type
G-type (Yellow (Sun-like))Distance from Star
4.03 AU (603 million km)Orbital Period
8.09 yearsAtmosphere
Hydrogen and helium dominated with trace methane and ammonia
Elemental Composition
H - Hydrogen
50.6%
He - Helium
18.4%
C - Carbon
7.4%
Surface Characteristics
No solid surface - thick gaseous envelope with possible rocky core deep withinClosest Real Exoplanet
Kepler-167 e87% similar
Orbiting Kepler-167| Yours | Kepler-167 e | |
|---|---|---|
| Mass | 300.0 × Earth | 321.0 × Earth |
| Radius | 10.8 × Earth | 10.2 × Earth |
| Density (composition) | 1.30 g/cm³ | 1.67 g/cm³ |
| Temperature | 144.7 K | 134.0 K |
| Starlight received | 0.06 × Earth | 0.10 × Earth |
| Star temperature | 5,600 K | 4,884 K |
MoonsLife may exist on a moon
Moon 1stable0.0022% - 5.4 radii
Small and distant: a quiet, stable companion.
Tidal braking locked the planet to its moon: one face forever moonward.
Moon 2recedingOcean world - life possibleWater ice0.25% - 12.2 radii
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
Tidal heat sustains a subsurface ocean over a rock seafloor: a strong candidate for life (Europa-like, 96/100).
Moon 3receding0.079% - 35.4 radii
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
Moon 4receding0.050% - 52.7 radii
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
Moon 5receding0.14% - 95.7 radii
Outside the synchronous orbit: slowly receding, like Luna (~cm per year).
Moon 6merged0.032% - 62.9 radii
Merged with an adjacent moon: too close for both to hold a stable orbit.
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